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neutronic [2014/06/12 18:35] yuan finalize wiki |
neutronic [2014/06/12 20:06] yuan cleanup |
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- | ===== Neutronic ===== | + | ====== Neutronic ====== |
- | ==== Abstract ==== | + | ===== Abstract ===== |
Modelling XRB nucleosynthesis in XNET following the model of the <del>Dissertation of Lau 2012</del> Fisker 2007, using the premade model for CNO XRB. | Modelling XRB nucleosynthesis in XNET following the model of the <del>Dissertation of Lau 2012</del> Fisker 2007, using the premade model for CNO XRB. | ||
- | Goal: Create video of working burst nuclides chart. Vary initial metallicity still using Fisker thermal trajectory, see if burst still occurs. Vary initial h/he ratio within metallicity still using Fisker thermal trajectory, see if burst still occurs. Create videos of stalled burst nuclides charts. | + | ===== Goals ===== |
- | ==== Log ==== | + | * Create video of working burst nuclides chart. |
+ | * Vary initial metallicity still using Fisker thermal trajectory, see if burst still occurs. | ||
+ | * Vary initial H/He ratio within metallicity still using Fisker thermal trajectory, see if burst still occurs. | ||
+ | * Create videos of stalled burst nuclides charts. | ||
- | == Tsunghan Yeh: Inputs == | + | ===== Links ===== |
- | * Read Paper | + | * [[https://github.com/xrf/talent-astro-proj2|Code]] |
- | * Create network list/sunet- use premade scenario following Fisker_2007 (see references) | + | * [[https://wikihost.nscl.msu.edu/talent/lib/exe/fetch.php?media=neutronic.pdf|Presentation]] |
- | * Temperature profile- use Fisker premade scenario | + | |
- | * Determine initial molar abundances to altar ab_XRB file | + | |
- | * PPT 3,4,7 | + | |
- | == Amber Lauer: Code == | + | ===== Results ===== |
- | * Read Paper | + | * [[http://youtu.be/pHKFIH-Llqo|Video 1 (small nuclear network)]] |
- | * Study Xnet: made a clearer set of instructions for running non-default library: [[https://docmgmt.nscl.msu.edu/share/proxy/alfresco/api/node/content/workspace/SpacesStore/7f083725-bf8b-4544-8bd6-0758dfe92545/reaction%20network%20instructions|rxn net instructions]], ran XRB-CNO example, MS Excel eats a space column about half way down the file, was causing burst plotting errors. | + | * [[http://youtu.be/uV3hGIiyVgc|Video 2 (large nuclear network)]] |
- | * Use scripts to make plots- | + | |
- | * abundance plots working | + | |
- | * easier in Excel | + | |
- | * animation script working | + | |
- | * PPT 2,5,6, references | + | |
- | == Fei Yuan: Analysis == | + | ===== Conclusion ===== |
- | * Read Paper | + | Since the initial X-ray burst is dependent on so few nuclei, almost no configuration can stop the burst behavior in a toy model. |
- | * Design end objective | + | |
- | * <del>Integrate the energy generated at the surface and compare to surface photon emission</del> (goal changed) | + | |
- | * vary metallicities to identify burst conditions (see abstract) | + | |
- | * refine python scripts to [[https://github.com/xrf/talent-astro-proj2/blob/master/tso_reader.py|read output]], visualize | + | |
- | * make video with [[https://github.com/xrf/talent-astro-proj2/blob/master/plot-chart|script]] | + | |
- | * PPT 8,9,10 | + | |
- | ==== Results ==== | + | ===== Log ===== |
- | * [[http://youtu.be/pHKFIH-Llqo|Video 1 (small nuclear network)]] | + | ==== Tsunghan Yeh: Inputs ==== |
- | * [[http://youtu.be/uV3hGIiyVgc|Video 2 (large nuclear network)]] | + | |
- | ==== Conclusion ==== | + | * Read paper |
+ | * Create network list/sunet: use premade scenario following Fisker_2007 (see references in presentation) | ||
+ | * Temperature profile: use Fisker premade scenario | ||
+ | * Determine initial molar abundances to alter ab_XRB file | ||
+ | * PPT 3, 4, 7 | ||
- | Since the initial X-ray burst is dependent on so few nuclei, almost no configuration can stop the burst behavior in a toy model. | + | ==== Amber Lauer: Code ==== |
- | ==== Links ==== | + | * Read paper |
+ | * Study Xnet: made a clearer set of instructions for running non-default library: [[https://docmgmt.nscl.msu.edu/share/proxy/alfresco/api/node/content/workspace/SpacesStore/7f083725-bf8b-4544-8bd6-0758dfe92545/reaction%20network%20instructions|rxn net instructions]], ran XRB-CNO example, MS Excel eats a space column about half way down the file, was causing burst plotting errors. | ||
+ | * Use scripts to make plots-: | ||
+ | * Abundance plots working | ||
+ | * Easier in Excel | ||
+ | * Animation script working | ||
+ | * PPT 2, 5, 6, references | ||
- | * [[https://github.com/xrf/talent-astro-proj2|Git repository]] | + | ==== Fei Yuan: Analysis ==== |
- | * [[https://github.com/xrf/talent-astro-proj2/raw/master/presentation.pdf|Presentation]] | + | |
+ | * Read paper | ||
+ | * Design end objective | ||
+ | * <del>Integrate the energy generated at the surface and compare to surface photon emission</del> (goal changed) | ||
+ | * vary metallicities to identify burst conditions (see abstract) | ||
+ | * Refine python scripts to [[https://github.com/xrf/talent-astro-proj2/blob/master/tso_reader.py|read output]], visualize | ||
+ | * Make video with [[https://github.com/xrf/talent-astro-proj2/blob/master/plot-chart|script]] | ||
+ | * PPT 8, 9, 10 | ||